Velocity Distribution Function of Gas Molecules

We finally get to handle something real — gases! Starting from a simple ideal gas model, we derive the velocity distribution using the Boltzmann distribution.

Up until now, we haven’t dealt with anything concrete. We’ve mostly been playing with numbers. What did they mean? Probabilities, more or less… haha.

But now we’re going to get our hands on something: gases!

Alright, to talk about gases, we need a model. Let’s make it a simple one. I’ll just list the assumptions.

  1. All the gas molecules are monatomic.
  2. We ignore rotational and vibrational energy for now.
  3. The molecules are ridiculously tiny. Basically points.
  4. Collisions between molecules are rare in this dilute model.
  5. There are no interactions such as gravity or electrical forces.
  6. The system is closed and kept at temperature $T$. Remember the canonical ensemble?

Oh my. All that just to say we’re only keeping translational kinetic energy?

We’ll apply the Boltzmann distribution to the gas in this model. That distribution was about energy, right? Since we’re only keeping kinetic energy, it is

Equation from the original notes

Let’s look at one component at a time, then put them all together. Here we go!

Equation from the original notes

For a molecule in this system at temperature $T$, write the probability density of its x-component of velocity, equation, as equation. The Boltzmann factor supplies the energy dependence:

Equation from the original notes

Put the x-component’s kinetic energy in the exponent, and we get

Equation from the original notes

Now what if we put $N$ gas molecules into that system?

The fraction per unit x-velocity at equation is proportional to

Equation from the original notes

Multiply by $N$ to get the number of molecules per unit x-velocity near equation:

Equation from the original notes

So that number-density expression is

Equation from the original notes

I don’t know what to call the proportionality constant, so as usual, let’s call it blah.

That leaves this density factor:

Equation from the original notes

Across all possible velocities, the total probability must be 1. We could list values such as

Equation from the original notes

and try adding the expressions:

Equation from the original notes

Ugh, let’s not do it that way. These are density values, and velocity is continuous, so we need an integral:

Equation from the original notes

How do we do this integral?

This is where the Gaussian integral comes in:

Equation from the original notes

Using it, with $\alpha=m/(2k_B T)$, gives

Equation from the original notes

Equation from the original notes

Yay! Now we’ve pinned down blah in the velocity distribution:

Equation from the original notes

We can give this whole expression a shorter name, equation.

In other words, equation is our normalized velocity probability density.

For $N$ molecules, the expected number with x-velocities between equation and $v_x+dv_x$ is $N g(v_x)\,dv_x$. The picture writes the number-density factor as equation; multiply it by the little interval width $dv_x$ to get an expected count.

Alright, we’re done exploring the x-component. What about y and z?

Ugh, apart from replacing equation with equation or equation, everything is the same, so the conclusions will be the same too.

Equation from the original notes

So here’s what we want to know next.

Of the $N$ molecules at temperature $T$, how many fall into small ranges around all three components of this velocity, equation?

Here’s how we’ll sift them out:

Equation from the original notes

First select the x-range, then the y-range within that group, then the z-range. That way, we account for every molecule in the little velocity box around equation.

The component distributions are independent in this model, so following the picture’s order gives this product:

Equation from the original notes

To turn the pictured density into an expected count, include all three interval widths, $dv_x\,dv_y\,dv_z$. Does that make sense? I hope so… heh.

By exactly the same logic as in the one-dimensional case, equation is the joint probability density that divides up our whole collection of $N$ molecules. Across all possible combinations, like these,

Equation from the original notes

The total probability must be 1. Velocity is continuous, so we integrate the density over all three components instead of adding isolated values:

Equation from the original notes

There we go. That does it!


Heads-up. The figures here are the original notes, slips and all. A few things to watch for:

  • In the Gaussian-integral picture, the exponent should be $-\alpha x^2$ and the upper limit $\infty$: $\int_{-\infty}^{\infty} e^{-\alpha x^2}\,dx = \sqrt{\pi/\alpha}$ (the picture writes $e^{-\alpha x}$ and “$=\infty$”). The next picture uses $e^{-\alpha v_x^2}$ correctly.
  • The pictures count “the molecules with velocity $v_x$” ($Ng(v_x)$ of them). Velocity is continuous, so strictly $g$ is a density: the expected number with an $x$-velocity between $v_x$ and $v_x + dv_x$ is $Ng(v_x)\,dv_x$.

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